Dark Matter Search Results from the PICO−60 C3F8 Bubble Chamber
| Autor: | T. Nania, M. Laurin, U. Chowdhury, G. Giroux, V. Zacek, Amber M. Ortega, O. Scallon, Eric W. Hoppe, W. H. Lippincott, J. Hall, M. Ardid, D. Baxter, G. Cao, P. Campion, J. Farine, Yongke Yan, I. Stekl, F. Mamedov, Satyajit Seth, A. E. Robinson, Deepam Maurya, A. Roeder, Jie Zhang, F. Tardif, P. S. Cooper, C. B. Krauss, S. Olson, Shashank Priya, H. Borsodi, F. Girard, C. E. Dahl, Ilan Levine, E. Vázquez-Jáuregui, J. I. Collar, R. Podviyanuk, O. Harris, J. Wells, R. Rucinski, Ivan Felis, R. Filgas, Manuel Bou-Cabo, G. Crowder, R. Neilson, C. Amole, N. Starinski, M. Jin, Karl J. Clark, Chujie Chen, I. Lawson, A. J. Noble, S. Fallows, A. Plante, D. M. Asner, Mala Das, Pijushpani Bhattacharjee, M. B. Crisler, I. J. Arnquist, U. Wichoski, P. Mitra, A. Sonnenschein, A. Leblanc, E. Behnke |
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| Rok vydání: | 2017 |
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| Zdroj: | Physical Review Letters. 118 |
| ISSN: | 1079-7114 0031-9007 |
| Popis: | The PICO Collaboration wishes to thank SNOLAB and its staff for support through underground space, logistical, and technical services. SNOLAB operations are supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site. We are grateful to Kristian Hahn and Stanislava Sevova of Northwestern University and Bjorn Penning of the University of Bristol for their assistance and useful discussion. We wish to acknowledge the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI) for funding. We acknowledge the support from National Science Foundation (NSF) (Grants No. 0919526, No. 1506337, No. 1242637, and No. 1205987). We acknowledge that this work is supported by the U.S. Department of Energy (DOE) Office of Science, Office of High Energy Physics (under Award No. DE-SC-0012161), by a DOE Office of Science Graduate Student Research (SCGSR) award, by Direccion General Asuntos del Personal Academico, Universidad Nacional Autonoma de Mexico (DGAPA-UNAM) through the grant Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPIIT) No. IA100316 and by Consejo Nacional de Ciencia y Tecnologia (CONACyT) (Mexico) through Grant No. 252167, by the Department of Atomic Energy (DAE), the Government of India, under the Center of AstroParticle Physics II project (CAPP-II) at Saha Institute of Nuclear Physics (SINP), by the Czech Ministry of Education, Youth and Sports (Grant No. LM2015072), and by the Spanish Ministerio de Economia y Competitividad, Consolider MultiDark (Grant No. CSD2009-00064). This work is partially supported by the Kavli Institute for Cosmological Physics at the University of Chicago through NSF Grant No. 1125897, and an endowment from the Kavli Foundation and its founder Fred Kavli. We also wish to acknowledge the support from Fermi National Accelerator Laboratory under Contract No. De-AC02-07CH11359, and Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. We also thank Compute Canada and the Center for Advanced Computing, ACENET, Calcul Quebec, Compute Ontario, and WestGrid for the computational support. |
| Databáze: | OpenAIRE |
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